Table 3
Physical properties derived from the integrated spectra of each H ii region.
Region | SFR | sSFR/L/L∗ | N2 | O3N2 | log U | E(B−V) |
(M⊙ yr-1) | (M⊙ yr-1) | 12 + log(O/H) | 12 + log(O/H) | (mag) | ||
|
||||||
H ii-1 | 0.26±0.01 | 0.56±0.15 | 8.54±0.16 | 8.53±0.18 | –3.35±0.01 | 0.37±0.03 |
H ii-2 | 0.56±0.02 | 0.73±0.15 | 8.54±0.16 | 8.57±0.18 | –3.58±0.01 | 0.46±0.03 |
H ii-3 | 0.41±0.01 | 0.41±0.17 | 8.52±0.16 | 8.56±0.18 | –3.46±0.01 | 0.41±0.01 |
H ii-4 | 0.22±0.01 | 0.42±0.14 | 8.49±0.16 | 8.45±0.18 | –3.35±0.01 | 0.30±0.03 |
H ii-5 | 1.43±0.02 | 2.67±0.36 | 8.48±0.16 | 8.41±0.18 | –3.01±0.01 | 0.22±0.03 |
H ii-6 | 0.25±0.03 | 0.96±0.23 | 8.49±0.16 | 8.42±0.18 | –3.10±0.01 | 0.16±0.03 |
H ii-7 | 0.78±0.02 | 1.93±0.30 | 8.50±0.16 | 8.41±0.18 | –2.99±0.01 | 0.24±0.03 |
Notes. The table lists: (Col. 2) the star formation rate and (Col. 3) the specific star formation rate per unit luminosity; (Cols. 4 and 5) the metallicity obtained with the N2 and the O3N2 indicators; (Col. 6) the ionisation parameter log U estimated using the [S ii] lines and the formulation given in Díaz et al. (2000), and (Col. 7) the estimate of the extinction E(B−V).
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